To demonstrate the capabilities of our improved algorithm to follow the serpentizination process we used the same setup as [1]}, but with the corrections listed above.
We consider the deepest 100 m radius, without taking other heat sources and heat/material transfer into account.
In each case the amount of non-reacting material of the test object was constant, 14% of the volume of planetesimals. We investigated how the different parameters of the model can influence the outcome compared with the [1]} results.
